The European Large Area ISO Survey VII: ROSAT observations of ELAIS sources
arXiv:astro-ph/0111407 · doi:10.1046/j.1365-8711.2002.05191.x
Abstract
We present a cross-correlation between the ELAIS 15m ISO survey with the {\it ROSAT} (0.1-2 keV) all-sky survey and the pointed observations WGACAT source catalogue. The resulting sample contains 15 objects. Optical spectroscopic identifications exist for 13 objects: 6 broad-line QSOs, 4 narrow line galaxies or type-2 AGN (NLG) and 3 stars. We have used both the X-ray to IR luminosity flux ratio and the X-ray hardness ratios diagnostics to estimate the amount of obscuration in these objects. The X-ray spectrum of the narrow-line galaxies does not present strong evidence for obscuration; however, the low ratio combined with the high X-ray luminosities suggest that at least one of the narrow line galaxies is associated with an obscured Seyfert nucleus. 4 out of 6 QSOs present high ratios and steep X-ray spectra with . One QSO (ELAISC15-J133442+375736) at a redshift of z=1.89, has an abnormally low X-ray/IR flux ratio, with its infrared luminosity approaching that of an hyperluminous galaxy (). Finally, one radio-loud QSO is the hardest X-ray source in our sample, presenting strong evidence for a high absorbing column ().
6 pages, 4 figures, in press MNRAS
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- XMM-Newton observations of the Lockman Hole V: time variability of the brightest AGN
- The Chandra Deep Field North Survey. VII. X-ray Emission from Lyman Break Galaxies
- The European Large Area ISO Survey V: a BeppoSAX hard X-ray survey of the S1 region
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- The European Large Area ISO Survey IX: the 90 micron luminosity function from the Final Analysis sample
- FIRBACK IV: Towards the nature of the 170microns source population
- AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South
- The AKARI FU-HYU galaxy evolution program: First results from the GOODS-N field
- An Overdensity of Extremely Red Objects Around Faint Mid-IR galaxies